Gulliver 46
0.12
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.5
Clit
0.16
Cdup
Stellar density (N50/rad)
36.0 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.5 Moderately studied
- Cdup 0.16 Likely duplicate
Overview
Gulliver 46 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 186.232 | -61.973 | 0.212 | -6.943 | 0.15 | -36.151 |
| Almeida et al. | 2025 | 186.244 | -61.974 | â | â | â | â |
| Celli et al. | 2024 | 186.234 | -61.973 | â | â | â | â |
| Cavallo et al. | 2024 | 186.262 | -61.98 | 0.216 | â | â | â |
| Hunt & Reffert | 2023 | 186.234 | -61.972 | 0.224 | -6.945 | 0.149 | -38.6 |
| Dias et al. | 2021 | 186.244 | -61.974 | 0.165 | -6.945 | 0.12 | -37.22 |
| Cantat-Gaudin et al. | 2020 | 186.234 | -61.973 | 0.181 | -6.946 | 0.125 | â |
| Cantat-Gaudin & Anders | 2020 | 186.234 | -61.973 | 0.181 | -6.946 | 0.125 | â |
| Monteiro & Dias | 2019 | 186.234 | -61.973 | â | â | â | 2.732 |
| Cantat-Gaudin et al. | 2018 | 186.234 | -61.973 | 0.181 | -6.946 | 0.125 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 4.295 | 2.65 | 2.58 | 26 | 0.035 | 606 | â | â |
| Almeida et al. | 2025 | 3.19 | 2.61 | â | 39 | â | 512 | â | â |
| Celli et al. | 2024 | â | â | â | 12 | â | 699 | â | â |
| Cavallo et al. | 2024 | 3.56 | 3.07 | â | 49 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 4.00 | 3.08 | 2.58 | 26 | â | â | â | â |
| Dias et al. | 2021 | 3.19 | 2.61 | â | 39 | 0.175 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.59 | 2.67 | â | 12 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.77 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 6.02 | 2.63 | â | 12 | 0.035 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.77 | â | â | â | â | â | â | â |
MOCA


Palma et al. (2025)
Classified as optical pair P396, along with HSC_2506.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.